EE549 - Power System Dynamics and Controlsiva/2021/ee549/Power_System_Stability...us understand the...

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Classical Model

In this model, the stability of a single generator connected to aninfinite bus is analyzed.

Though this model is not suitable for current power systems, it helpsus understand the basic phenomenon of stability.

Assumptions

1 Exciter dynamics are neglected and the filed current is assumed to beconstant so that the induced voltage is always constant.

2 Damper winding dynamics are neglected.

3 The mechanical input power is assumed to be constant during theperiod of study.

4 Rotor is assumed to be of cylindrical type so that no saliency ispresent.

Siva (IIT P) EE549 1 / 61

SMIB System

Let us consider Single Machine Infinite Bus (SMIB) system.

E δ V∞ = 1∠0◦

Pe =EV sin δ

X

Where X = Xg + XTr + XTL in p.u.

Siva (IIT P) EE549 2 / 61

Rotor Dynamics - Swing EquationThe equation governing rotor motion of a synchronous machine is given as

Jd2θmdt2

= Ta = Tm − Te N-m

whereJ = the total moment of inertia of the rotor masses in kg-m2

θm = the angular displacement of the rotor with respect to a stationaryaxis in mechanical radians (rad)t = time in seconds (s)Tm = the mechanical or shaft torque supplied by the prime mover in N-mTe = the net electrical or electromagnetic torque in N-mTa = the net accelerating torque in N-m

Siva (IIT P) EE549 3 / 61

Tm and Te are considered positive for the synchronous generator.

Tm accelerates the rotor in the positive θm in the direction of rotation.

For a motor, Tm and Te are reversed in sign.

In the steady state, Tm = Te . Hence, Ta = 0.

θm is measured with respect to a stationary reference axis on the stator. Torepresent it with respect to the synchronously rotating frame, let us define

θm = ωsmt + δm

whereωsm is the synchronous speed of the machine in mechanical radians persecondδm is the angular displacement of the rotor in mechanical radians from thesynchronously rotating reference axis.

Siva (IIT P) EE549 4 / 61

dθmdt

= ωsm +dδmdt

ωm − ωsm =dδmdt

where ωm =dθmdt

is the angular velocity of the rotor in mechanical radians

per second.Differentiating it again,

d2θmdt2

=d2δmdt2

Substituting it,

Jd2δmdt2

= Ta = Tm − Te N-m

On multiplying by ωm,

Jωmd2δmdt2

= Pa = Pm − Pe

Siva (IIT P) EE549 5 / 61

wherePm = shaft power input in MWPe = electrical power output in MWPa = accelerating power in MW

Let us define inertia constant H.

H =stored kinetic energy in megajoules at synchronous speed

Machine rating in MVA

H =12Jω

2sm

SmachMJ/MVA

Substituting it,2H

ω2sm

ωmd2δmdt2

=Pa

Smach=

Pm − Pe

Smach

In practice, ωm does not differ significantly from the synchronous speed.ωm ≈ ωsm

2H

ωsm

d2δmdt2

= Pa = Pm − Pe per unit

Siva (IIT P) EE549 6 / 61

It can be written as

2H

ωs

d2δ

dt2= Pm − Pe per unit

δ and ωs have consistent units which can be mechanical or electricaldegrees or radians.

This equation is called the swing equation of the machine.

It is a second-order nonlinear differential equation.

When it is solved, we obtain δ as a function of t. This is called theswing curve.

Siva (IIT P) EE549 7 / 61

It can be written as two first-order differential equations.

2H

ωs

dt= Pm − Pe per unit

dt= ω − ωs

ω, ωs and δ involve electrical radians or electrical degrees.

δ is the load angle.

Siva (IIT P) EE549 8 / 61

Small Signal Stability

δ

P

Pm

Pmax

δ0 δmax

Consider small incremental changes in δ around δ0. The swing equationcan be expressed as follows:

2H

ωs

d2(δ0 + ∆δ)

dt2= Pm − Pmax sin(δ0 + ∆δ)

2H

ωs

d2δ0dt2

+2H

ωs

d2∆δ

dt2= Pm − Pmax sin δ0 cos ∆δ − Pmax cos δ0 sin ∆δ

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Since ∆δ is very small,

sin ∆δ ≈ ∆δ; cos ∆δ ≈ 1

2H

ωs

d2δ0dt2

+2H

ωs

d2∆δ

dt2= Pm − Pmax sin δ0 − Pmax cos δ0∆δ

At the stable equilibrium point (δ0),

2H

ωs

d2δ0dt2

= Pm − Pmax sin δ0 = 0

Therefore,2H

ωs

d2∆δ

dt2= −Pmax cos δ0∆δ

Let Ps = Pmax cos δ0. Ps is called the synchronizing power or torque. Inper unit system, torque and power are equal.

2H

ωs

d2∆δ

dt2+ Ps∆δ = 0

Siva (IIT P) EE549 10 / 61

It is a linear second-order differential equation.

When Ps is positive, the solution ∆δ(t) is an undamped sinusoid.

When Ps is negative, the solution ∆δ(t) increases exponentiallywithout limit.

Ps is positive at δ0 and negative at δmax .

Therefore δ0 is a stable equilibrium point and δmax is an unstableequilibrium point.

Siva (IIT P) EE549 11 / 61

Let us apply the Laplace transformation to it.

2H

ωss2∆δ(s) + Ps∆δ(s) = 0

On solving, we get two roots.

s = ±√−Psωs

2H

If Ps is positive,

s = ±√

Psωs

2H

The system has sustained oscillation. It is marginally stable.If Ps is negative,

s = +

√Psωs

2H,−√

Psωs

2H

The system is unstable.

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In synchronous machines, damper or amortisseur windings are there.

1 They damp out oscillations in generators.

2 They help synchronous motors start as induction motors becausesynchronous motors do not have starting torque.

The damping torque depends on the rate change of rotor angle.

Pd = Ddδ

dt

where D is the damping coefficient. After including this, the linearizedswing equation can be written as

2H

ωs

d2∆δ

dt2+ D

d∆δ

dt+ Ps∆δ = 0

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Applying the Laplace transformation,

2H

ωss2∆δ(s) + Ds∆δ(s) + Ps∆δ(s) = 0

s2 +ωs

2HDs +

ωs

2HPs = 0

By comparing this with the standard characteristics equation of a secondorder system,

s2 + 2ζωns + ω2n = 0

we get

ωn =

√ωs

2HPs

ζ =D

2

√ωs

2HPs

where ωn is the natural frequency of oscillations and ζ is the dampingratio.

Siva (IIT P) EE549 14 / 61

The roots (eigen values) of the characteristics equation are

s = −ζωn ± ωn

√1− ζ2

If Ps is positive

there will be two complex conjugate roots with negative real part.

hence the system will be stable.

If Ps is negative,

there will be two real roots with one positive.

hence the system will be unstable.

Siva (IIT P) EE549 15 / 61

The linearized swing equations can also be written as follows:

2H

ωs

d∆ω

dt+ D∆ω + Ps∆δ = 0

d∆δ

dt= ∆ω

In state space form,[∆ω̇

∆δ̇

]=

[−ωsD

2H−ωsPs

2H1 0

] [∆ω∆δ

]By taking the Laplace transformation,[

s∆ω(s)−∆ω(0)s∆δ(s)−∆δ(0)

]=

[−ωsD

2H−ωsPs

2H1 0

] [∆ω(s)∆δ(s)

]

Siva (IIT P) EE549 16 / 61

[∆ω(s)∆δ(s)

]=

[s +

ωsD

2H

ωsPs

2H−1 s

]−1 [∆ω(0)∆δ(0)

]This can be written as[

∆ω(s)∆δ(s)

]=

[s + 2ζωn ω2

n

−1 s

]−1 [∆ω(0)∆δ(0)

]If the rotor angle is perturbed by a small angle, ∆δ(0) = ∆δ and∆ω(0) = 0.

∆ω(s) = − ω2n∆δ

s2 + 2ζωns + ω2n

∆δ(s) =(s + 2ζωn)∆δ

s2 + 2ζωns + ω2n

Siva (IIT P) EE549 17 / 61

By taking the inverse Laplace transformation, we can get the following.

∆ω(t) = − ωn∆δ√1− ζ2

e−ζωnt sinωd t

and

∆δ(t) =∆δ√1− ζ2

e−ζωnt sin(ωd t + θ)

where ωd = ωn

√1− ζ2 and θ = cos−1(ζ).

The motion of rotor relative to the operating point is

δ = δ0 +∆δ√1− ζ2

e−ζωnt sin(ωd t + θ)

and the rotor angular frequency is

ω = ω0 −ωn∆δ√1− ζ2

e−ζωnt sinωd t

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The time constant is

τ =1

ζωn

τ =4H

ωsD

The response approximately settles at 4 to 5 time constants.

As H increase, it results in a longer settling time.

As Ps increases, it results in an increase in ωn.

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Example

A 50 Hz synchronous generator having inertia constant H = 5 sec and adirect axis reactance X ′d = 0.3 p.u. is connected to an infinite bus througha transformer and a double circuit line. The network is purely reactive. Thesynchronous generator is delivering real power P = 0.8 p.u. and reactivepower Q = 0.074 p.u. to the infinite bus of 1.0 p.u at steady state.

0.2

E ′d

X ′d = 0.3

V∞ = 1∠0◦

X = 0.3

X = 0.3

Assume the per unit damping power coefficient D = 0.2. Consider a smalldisturbance of ∆δ = 10◦. For example, the breakers open and quickly close.Determine the motion of rotor angle and the generator frequency.

Siva (IIT P) EE549 20 / 61

The current flowing into the infinite bus is

I =S∗

V ∗=

0.8− 0.074

1∠0◦= 0.8− 0.074

The reactance between E ′d and V∞ before the fault is

X = 0.3 + 0.2 +0.3 + 0.3

2= 0.65

The direct axis transient internal voltage is

E ′d = V∞ + X1I = 1∠0◦ + 0.65× (0.8− 0.074) = 1.17∠26.38◦

Pmax =E ′dV∞X1

=1.17× 1

0.65= 1.8

δ0 = 26.38◦

Siva (IIT P) EE549 21 / 61

Ps = Pmax cos δ0 = 1.8× cos(26.38◦) = 1.6125

ωn =

√ωs

2HPs = 7.1174 rad/s

fn = 1.133 Hz

ζ =D

2

√ωs

2HPs= 0.4414

ωd = ωn

√1− ζ2 = 6.3866 rad/s

θ = cos−1 ζ = 92.4◦

δ = 26.38◦ + 11.1444e−3.1416t sin(6.4t + 92.4◦)

f = 50− 0.2525e−3.1416t sin 6.4t

Siva (IIT P) EE549 22 / 61

t (s)

δ (deg)

26.38◦

Figure: Swing Curve

t (s)

f (Hz)

50

Figure: Frequency

Siva (IIT P) EE549 23 / 61

Transient Stability

The stability of a system is analyzed when it is subjected to largedisturbances like faults.

Since the disturbances are large, the rotor angle will swing high.

This does not let us linearize the swing equation.

The analysis of large disturbance stability is difficult.

The equation has to be solved using numerical integration techniques.

However, for an SMIB system, a direct approach called Equal AreaCriterion method can be used to analyze it.

It is a graphical approach.

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Equal Area Criterion

2H

ωs

d2δ

dt2= Pm − Pe

d2δ

dt2=ωs

2H(Pm − Pe)

Let us multiply both sides of the above equation by 2dδ/dt,

2dδ

dt

d2δ

dt2=ωs(Pm − Pe)

H

dt

d

dt

[dδ

dt

]2=ωs(Pm − Pe)

H

dt

On integration, [dδ

dt

]2=

∫ δm

δ0

ωs(Pm − Pe)

Hdδ

Siva (IIT P) EE549 25 / 61

For a system to be stable,dδ

dt= 0 after a disturbance.

∫ δm

δ0

ωs(Pm − Pe)

Hdδ = 0

∫ δm

δ0

(Pm − Pe)dδ = 0

where

δ0 = initial rotor angle

δm = maximum rotor angle

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Sudden change in Pm

δ

P

Pm0

Pm1

Pmax

δ0δ1δm

Siva (IIT P) EE549 27 / 61

∫ δm

δ0

(Pm1 − Pe)dδ = 0

δ0 is the initial rotor angle. δm is the maximum rotor angle duringoscillation. ∫ δ1

δ0

(Pm1 − Pe)dδ +

∫ δm

δ1

(Pm1 − Pe)dδ = 0

∫ δ1

δ0

(Pm1 − Pe)dδ =

∫ δm

δ1

(Pe − Pm1)dδ

Therefore for the system to be stable

Area(A1) = Area(A2)

Energy Gained = Energy Lost

If A1 > A2, the system will be unstable.

Siva (IIT P) EE549 28 / 61

t

δδm

δ0

δ1

Figure: Swing Curve

Damper or amortisseur windings damp out oscillations.

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Short Circuit Faults

E δ V∞ = 1∠0◦

F

At point F , a three phase fault occurs. To analyze this, we need tounderstand the physical conditions before, during and after the fault.

Siva (IIT P) EE549 30 / 61

1 Before Fault :

−+

E δ

X ′d XTr

−+

1∠0◦

XTL

XTL

X1 = X ′d + XTr +XTL

2

Pe1 = Pmax1 sin δ

where

Pmax1 =EV

X1

Siva (IIT P) EE549 31 / 61

2 During Fault :

−+

E δ

X ′d XTr

−+

1∠0◦

XTL

XTL2

XTL2

The total reactance X between two nodes can be found using Y −∆conversion.X2 during fault will be higher than before fault X1.

Hence,

Pe2 = Pmax2 sin δ

where

Pmax2 =EV

X2

Siva (IIT P) EE549 32 / 61

3 After Fault :

−+

E δ

X ′d XTr

−+

1∠0◦

XTL

X3 = X ′d + XTr + XTL

Pe3 = Pmax3 sin δ

where

Pmax3 =EV

X3

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δ

P

Pm

Pmax1

Pmax3

Pmax2

δ0 δcr δmax

A1

A2

δmax = π − sin−1( PmPmax3

).For the system to be stable, A1 = A2. There is a critical clearing angle δcrbefore which the fault has to be cleared.∫ δcr

δ0

(Pm − Pmax2 sin δ)dδ =

∫ δmax

δcr

(Pmax3 sin δ − Pm)dδ

Siva (IIT P) EE549 34 / 61

Integrating and simplifying the above equation, we get

cos δcr =Pm(δmax − δ0) + Pmax3 cos δmax − Pmax2 cos δ0

(Pmax3 − Pmax2)

t

δ

δm

δcr

tcr

δ0

Figure: Swing Curve

tcr is the critical clearing time in seconds.It will settle at δnew = sin−1( Pm

Pmax3) if damping is present.

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Short Circuit Faults at the end of Transmission Lines(Near the bus)

E δ V∞ = 1∠0◦

F

1 Before Fault :

X1 = X ′d + XTr +XTL

2

Pe1 = Pmax1 sin δ

where

Pmax1 =EV

X1

Siva (IIT P) EE549 36 / 61

2 During Fault :

Since the fault is near the bus, the bus voltage is zero.The power transfer during fault is zero.

Hence,

Pe2 = 0

3 After Fault :

X3 = X ′d + XTr + XTL

Pe3 = Pmax3 sin δ

where

Pmax3 =EV

X3

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δ

P

Pm

Pmax1

Pmax3

δ0 δcr δmax

A1

A2

δmax = π − sin−1( PmPmax3

).For the system to be stable, A1 = A2.∫ δcr

δ0

Pmdδ =

∫ δmax

δcr

(Pmax3 sin δ − Pm)dδ

Siva (IIT P) EE549 38 / 61

Integrating and simplifying the above equation, we get

cos δcr =Pm(δmax − δ0) + Pmax3 cos δmax

Pmax3

We can find the critical clearing time for this case as follows:

d2δ

dt2=ωs

2H(Pm − Pe)

Since Pe = 0 during fault,

d2δ

dt2=ωs

2HPm

Integrating this,dδ

dt=

∫ t

0

ωs

2HPm =

ωs

2HPmt

On further integration,

δ =ωs

4HPmt

2 + δ0

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If δ = δcr ,

δcr =ωs

4HPmt

2cr + δ0

tcr =

√4H(δcr − δ0)

ωsPm

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Factors Influencing Transient Stability

1 How heavily the generator is loaded.

2 The generator output during the fault. This depends on the faultlocation and type.

3 The fault-clearing time.

4 The post fault transmission system reactance.

5 The generator inertia. The higher the inertia, the slower the rate ofchange in angle. This reduces A1.

6 The generator internal voltage magnitude E . This depends on thefield excitation.

Siva (IIT P) EE549 41 / 61

Numerical Integration Methods

Letdx

dt= f(x, t)

where x is the state vector and f(x, t) is a vector of non linear functions.1 Explicit Methods

1 Euler Method2 Modified Euler Method3 Runge-Kutta Methods

2 Implicit Methods1 Trapezoidal Rule

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Euler Method

Consider the first-order differential equation.

dx

dt= f (x , t)

with x = x0 at t = t0.

t

x

x0

t0

x1

t1

∆x ∆t

Siva (IIT P) EE549 43 / 61

At x = x0, t = t0, the curve can be approximated by its tangent having aslope

dx

dt

∣∣∣∣x=x0

= f (x0, t0)

Therefore,

∆x =dx

dt

∣∣∣∣x=x0

∆t

The value of x at t = t1 = t0 + ∆t is given by

x1 = x0 + ∆x = x0 +dx

dt

∣∣∣∣x=x0

∆t

This has to be repeated till the time reaches the final simulation time.

Since it considers only the firs derivative of x , it is referred to as afirst order method.

∆t has to be small to achieve accuracy.

Since it uses only the first order information, it may introduce error.

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Modified Euler Method

The standard Euler method results in inaccuracies because it uses thederivative at the beginning of the interval.

The modified Euler method tries to overcome this issue by using theaverage of the derivatives at the two ends.

It consists of the following steps.

1 Predictor step

xp1 = x0 +dx

dt

∣∣∣∣x=x0

∆t

2 Corrector step

xc1 = x0 +1

2

(dx

dt

∣∣∣∣x=x0

+dx

dt

∣∣∣∣x=xp1

)∆t

This process has to be repeated until the desired accuracy or the finalsimulation time.

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Runge-Kutta (R-K) Methods

Euler and the modified Euler method require smaller time steps.

R-K methods approximate the Taylor series solution. However they donot need derivatives higher than the first.

R-K methods use the effectiveness of higher derivatives by severalevaluations of the first derivative.

They are classified based on the number of evaluations.

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Second order R- K Method

The value of x at t = t0 + ∆t is

x1 = x0 + ∆x = x0 +k1 + k2

2

wherek1 = f (x0, t0)∆t

k2 = f (x0 + k1, t0 + ∆t)∆t

In general,

xn+1 = xn +k1 + k2

2

wherek1 = f (xn, tn)∆t

k2 = f (xn + k1, tn + ∆t)∆t

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Fourth order R- K Method

The value x at n + 1st step is

xn+1 = xn +1

6(k1 + 2k2 + 2k3 + k4)

wherek1 = f (xn, tn)∆t

k2 = f (xn +k12, tn +

∆t

2)∆t

k3 = f (xn +k22, tn +

∆t

2)∆t

k4 = f (xn + k3, tn + ∆t)∆t

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k1 = (slope at the beginning of time step)∆t

k2 = (first approximation to slope at mid step)∆t

k3 = (second approximation to slope at mid step)∆t

k4 = (slope at the end of step)∆t

∆x =1

6(k1 + 2k2 + 2k3 + k4)

This is equivalent to considering upto fourth derivative terms in the Taylorseries expansion.

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Stability of Explicit Methods

Explicit methods calculate x at any time step from the knowledge of thevalues of x at previous time steps.

They are not numerically stable.

They require smaller time steps.

For the stiff systems (Stiffness is the ratio of the largest to smallesttime constants), they blow up unless a small time step is used.

Stiffness can also be found by the ratio of the largest to smallesteigenvalues of the linearized system.

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Implicit Methods

Consider the differential equation

dx

dt= f (x , t)

with x = x0 and t = t0.

x1 = x0 +

∫ t1

t0

f (x , τ)dτ

Implicit methods approximate the integral.

The simplest implicit integration method is the trapezoidal rule.

The trapezoidal rule approximates the integral by trapezoids.

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Trapezoidal Rule

t

f (x , t)

f (x0, t0)

f (x1, t1)

t1∆tt0

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The trapezoidal rule is

x1 = x0 +∆t

2[f (x0, t0) + f (x1, t1)]

In general

xn+1 = xn +∆t

2[f (xn, tn) + f (xn+1, tn+1)]

xn+1 appears on both sides.

Implicit methods find x using x at the previous time step as well ascurrent value.

Since the current value is unknown, an implicit equation must besolved.

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Stability of Implicit Methods

Implicit methods are numerically stable

For the stiff systems, implicit methods suffer from accuracy but notnumerical stability.

Implicit methods work well with larger time steps.

For systems where time steps are limited by numerical stability ratherthan accuracy, implicit methods are better.

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Example

A 50 Hz synchronous generator having inertia constant H = 5 sec and adirect axis reactance X ′d = 0.3 p.u. is connected to an infinite bus througha transformer and a double circuit line. The network is purely reactive. Thesynchronous generator is delivering real power P = 0.8 p.u. and reactivepower Q = 0.074 p.u. to the infinite bus of 1.0 p.u at steady state.

0.2

E ′d

X ′d = 0.3

V∞ = 1∠0◦

X = 0.3

X = 0.3F

A solid three phase fault occurs at point F and the fault is cleared by openingthe faulted line.

1 Determine the critical clearing angle and the critical fault clearingtime using numerical integration.

2 Check the above angle using the Equal Area Criterion.

Siva (IIT P) EE549 55 / 61

The current flowing into the infinite bus is

I =S∗

V ∗=

0.8− 0.074

1∠0◦= 0.8− 0.074

The reactance between E ′d and V∞ before the fault is

X1 = 0.3 + 0.2 +0.3 + 0.3

2= 0.65

The direct axis transient internal voltage is

E ′d = V∞ + X1I = 1∠0◦ + 0.65× (0.8− 0.074) = 1.17∠26.38◦

Pmax1 =E ′dV∞X1

=1.17× 1

0.65= 1.8

δ0 = 26.38◦

Siva (IIT P) EE549 56 / 61

The reactance during the fault is

X2 =∞

Pmax2 = 0

The reactance after the fault is

X3 = 0.3 + 0.2 + 0.3 = 0.8

Pmax3 =1.17× 1

0.8= 1.46

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The swing equation can be written as follows:

dt=ωs

2H(Pm − Pe)

dt= (ω − ωs)

The general formula for the second order R-K method

ωn+1 = ωn +

(k1ω + k2ω

2

)δn+1 = δn +

(k1δ + k2δ

2

)where

k1ω =ωs

2H(Pm − Pmax sin(δn))∆t

k1δ = (ωn − ωs)∆t

k2ω =ωs

2H(Pm − Pmax sin(δn + k1ω))∆t

k2δ = (ωn + k1δ − ωs)∆t

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Figure: Swing Curve

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The fault was applied at t = 1 sec.

∆t = 0.05 sec.

The simulation was carried till tf = 5 sec.

It is found that the critical clearing time tcr = 0.2 sec.

δcr =ωs

4HPmt

2cr + δ0

δcr ≈ 55◦

By using the equal area criterion

cos δcr =Pm(δmax − δ0) + Pmax3 cos δmax

Pmax3

Pmax3 = 1.4625

δmax = π − sin−1(Pm

Pmax3) = 2.3887

δcr ≈ 54◦

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Drawbacks of the classical model

1 The dynamics of rotor field winding and the damper winding on thegenerator are totally neglected in the classical model. However, theycan effect the stability of a system significantly.

2 In the classical model, the internal voltage behind the transient reac-tance was assumed to be constant. This is not true since the rotorfiled current is controlled through an exciter and automatic voltageregulator (AVR). Their dynamics have to be included.

3 In the classical model, Pm is assumed to be constant. But Pm dependson speed governor and turbine dynamics. Their dynamics need to beconsidered.

4 Dynamic loads like induction motors, synchronous motors, power elec-tronic devices do affect the stability. In the classical model, they werenot taken into consideration.

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